Ambidextrous light transforms for celestial amplitudes

Abstract Low multiplicity celestial amplitudes of gluons and gravitons tend to be distributional in the celestial coordinates z, z ¯ $$ \overline{z} $$ . We provide a new systematic remedy to this situation by studying celestial amplitudes in a basis of light transformed boost eigenstates. Motivated...

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Main Author: Atul Sharma
Format: Article
Language:English
Published: SpringerOpen 2022-01-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP01(2022)031
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author Atul Sharma
author_facet Atul Sharma
author_sort Atul Sharma
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description Abstract Low multiplicity celestial amplitudes of gluons and gravitons tend to be distributional in the celestial coordinates z, z ¯ $$ \overline{z} $$ . We provide a new systematic remedy to this situation by studying celestial amplitudes in a basis of light transformed boost eigenstates. Motivated by a novel equivalence between light transforms and Witten’s half-Fourier transforms to twistor space, we light transform every positive helicity state in the coordinate z and every negative helicity state in z ¯ $$ \overline{z} $$ . With examples, we show that this “ambidextrous” prescription beautifully recasts two- and three-point celestial amplitudes in terms of standard conformally covariant structures. These are used to extract examples of celestial OPE for light transformed operators. We also study such amplitudes at higher multiplicity by constructing the Grassmannian representation of tree-level gluon celestial amplitudes as well as their light transforms. The formulae for n-point N k−2MHV amplitudes take the form of Euler-type integrals over regions in Gr(k, n) cut out by positive energy constraints.
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spelling doaj.art-e4261958a6134da48d0c2bd0975330752022-12-22T04:09:18ZengSpringerOpenJournal of High Energy Physics1029-84792022-01-012022113110.1007/JHEP01(2022)031Ambidextrous light transforms for celestial amplitudesAtul Sharma0The Mathematical Institute, University of OxfordAbstract Low multiplicity celestial amplitudes of gluons and gravitons tend to be distributional in the celestial coordinates z, z ¯ $$ \overline{z} $$ . We provide a new systematic remedy to this situation by studying celestial amplitudes in a basis of light transformed boost eigenstates. Motivated by a novel equivalence between light transforms and Witten’s half-Fourier transforms to twistor space, we light transform every positive helicity state in the coordinate z and every negative helicity state in z ¯ $$ \overline{z} $$ . With examples, we show that this “ambidextrous” prescription beautifully recasts two- and three-point celestial amplitudes in terms of standard conformally covariant structures. These are used to extract examples of celestial OPE for light transformed operators. We also study such amplitudes at higher multiplicity by constructing the Grassmannian representation of tree-level gluon celestial amplitudes as well as their light transforms. The formulae for n-point N k−2MHV amplitudes take the form of Euler-type integrals over regions in Gr(k, n) cut out by positive energy constraints.https://doi.org/10.1007/JHEP01(2022)031Gauge-gravity correspondenceScattering AmplitudesConformal Field Theory
spellingShingle Atul Sharma
Ambidextrous light transforms for celestial amplitudes
Journal of High Energy Physics
Gauge-gravity correspondence
Scattering Amplitudes
Conformal Field Theory
title Ambidextrous light transforms for celestial amplitudes
title_full Ambidextrous light transforms for celestial amplitudes
title_fullStr Ambidextrous light transforms for celestial amplitudes
title_full_unstemmed Ambidextrous light transforms for celestial amplitudes
title_short Ambidextrous light transforms for celestial amplitudes
title_sort ambidextrous light transforms for celestial amplitudes
topic Gauge-gravity correspondence
Scattering Amplitudes
Conformal Field Theory
url https://doi.org/10.1007/JHEP01(2022)031
work_keys_str_mv AT atulsharma ambidextrouslighttransformsforcelestialamplitudes